The Structure of the Atmosphere of Saturn at Mid-latitudes from Cassini Radio Occultations

Details The Structure of the Atmosphere of Saturn at Mid-latitudes from Cassini Radio Occultations The Structure of the Atmosphere of Saturn at Mid-latitudes from Cassini Radio Occultations

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008dps....40.4303s&link_type=abstract

American Astronomical Society, DPS meeting #40, #43.03; Bulletin of the American Astronomical Society, Vol. 40, p.475

Astronomy and Astrophysics

Astronomy

1

Scientific paper

A series of 11 radio occultations beginning in December 2007 and concluding July 2008 probed the atmosphere of Saturn at mid-latitudes. Four covered northern latitudes from 18 - 33 degrees, and 7 covered southern latitudes from 20 - 70 degrees. We present the temperature - pressure profiles obtained from the radio occultation data for this series of occultations, and compare them to previous Cassini and Voyager occultations which probed the same latitude range.

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